Skip to main content

Unlike the terrestrial planets, Jupiter and Saturn exhibit differential rotation, See Why...

Observations of features like the Great Red Spot and smaller
storms allow astronomers to determine how rapidly Jupiter and
Saturn rotate. At its equator, Jupiter completes a full rotation in
only 9 hours, 50 minutes, and 28 seconds, making it not only the
largest and most massive planet in the solar system but also the
one with the fastest rotation. However, Jupiter rotates in a strikingly
different way from the Earth, the Moon, Mercury, Venus,
or Mars.

Differential Rotation:

If Jupiter were a solid body like a terrestrial planet (or, for that
matter, a billiard ball), all parts of Jupiter’s surface would rotate
through one complete circle in this same amount of time (Figure
12-3a). But by watching features in Jupiter’s cloud cover, Gian
Domenico Cassini discovered in 1690 that the polar regions of
the planet rotate a little more slowly than do the equatorial regions.
(You may recall this Italian astronomer from Section 11-2
as the gifted observer who first determined Mars’s rate of rotation.)
Near the poles, the rotation period of Jupiter’s atmosphere
is about 9 hours, 55 minutes, and 41 seconds. Saturn, too, has alonger rotation period near its poles (10 hours, 39 minutes, and
24 seconds) than at its equator (10 hours, 13 minutes, and
59 seconds).


Comments

Popular posts from this blog

The Ptolemaic System

Explaining the nonuniform motions of the five planets was one of the main challenges facing the astronomers of antiquity. The Greeks developed many theories to account for retrograde motion and the loops that the planets trace out against the background stars. One of the most successful and enduring models was originated by Apollonius of Perga and by Hipparchus in the second century B.C. and expanded upon by Ptolemy, the last of the great Greek astronomers, during the second century A.D.  sketches the basic concept, usually called the Ptolemaic system. Each planet is assumed to move in a small circle called an epicycle, whose center in turn moves in a larger circle, called a deferent, which is centered approximately on the Earth. Both the epicycle and deferent rotate in the same direction As viewed from Earth, the epicycle moves eastward along the deferent. Most of the time the eastward motion of the planet on its epicycle adds to th...

Lorentz transformation

Lorentz transformation and its inverse : Define an event to have spacetime coordinates  ( t , x , y , z )  in system  S  and  ( t ′, x ′, y ′, z ′)  in a reference frame moving at a velocity v with respect to that frame,  S ′. Then the Lorentz transformation specifies that these coordinates are related in the following way: {\displaystyle {\begin{aligned}t'&=\gamma \ (t-vx/c^{2})\\x'&=\gamma \ (x-vt)\\y'&=y\\z'&=z,\end{aligned}}} where {\displaystyle \gamma ={\frac {1}{\sqrt {1-{\frac {v^{2}}{c^{2}}}}}}} is the Lorentz factor and  c  is the speed of light in vacuum, and the velocity  v  of  S ′, relative to  S , is parallel to the  x -axis. For simplicity, the  y  and  z  coordinates are unaffected; only the  x  and  t  coordinates are transformed. These Lorentz transformations form a one-param...

Special Theory Of Relativity

The theory of special relativity explains how space and time are linked for objects that are moving at a consistent speed in a straight line. One of its most famous aspects concerns objects moving at the speed of light.  Simply put, as an object approaches the speed of light, its mass becomes infinite and it is unable to go any faster than light travels. This cosmic speed limit has been a subject of much discussion in physics, and even in science fiction, as people think about how to travel across vast distances. The theory of special relativity was developed by Albert Einstein in 1905, and it forms part of the basis of modern physics. After finishing his work in special relativity, Einstein spent a decade pondering what would happen if one introduced acceleration. This formed the basis of his general relativity, published in 1915. Einstein's work led to some startling results, which today still seem counterintuitive at first glance even though his...